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History of Astronomy

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History of Astronomy Chapter 2 Apparent motion of stars Rise from east, and set in the west. Rotate around Polaris. Any star rises 3 min 56 sec earlier every night. – PowerPoint PPT presentation

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Title: History of Astronomy


1
History of Astronomy
  • Chapter 2

2
Apparent motion of stars
  • Rise from east, and set in the west.
  • Rotate around Polaris.
  • Any star rises 3 min 56 sec earlier every night.

3
Apparent motion of the Sun
  • Sun follows the ecliptic.
  • Ecliptic the path followed by the sun.

4
The celestial sphere ????? ????????
  • Zenith The point directly overhead.

5
Sunrise and sunset
6
Sunrise 28 Jan. 2012 (Dhahran)
7
Constellations ???????
  • Patterns of stars in the sky.
  • 88 constellations.
  • Served as a calendar.
  • Some imagination.
  • No physical relation
  • between members
  • of any constellation.

8
Zodiac circle of animals ????? ??????
9
Zodiac a band in which planets move.
10
Motion of planets
  • Follow the ecliptic.
  • Retrograde motion apparent reverse of planets
    motion.

11
Motion of the Moon
  • Follows the ecliptic in the sky.
  • Moonrise is 50 min late every night.
  • Moons shape changes because we see different
    amounts of its illuminated parts.

12
Eclipses
  • The angle between the moons orbit to the
    ecliptic plane is 5.15.
  • Eclipses do not occure every month.

13
Eclipses
  • Twice a year on average.
  • New moon (Solar eclipse)
  • Full moon (Lunar Eclipse)

14
2.1 Egyptian and Other Early Astronomy
  • River Nile floods every summer.
  • Relation to the first appearance of Sirius in
    the eastern sky before sunrise in early July.

15
2.2 Greek Astronomy
  • Prograde motion the ordinary direction of motion
    of planets (the same as the sun and the moon wrt
    stars).
  • Retrograde motion the apparent backward motion
    of planets wrt to stars.
  • Periods of retrograde motion ? Order of distance
    of planets

16
2.2 Greek Astronomy
  • Aristotle geocentric model

17
2.2 Greek Astronomy
  • Ptolemy epicycle, defernt, equant.

18
Problems With the Geocentric Model
  • The planets appear to change brightness, implying
    a change of distance.
  • The planets undergo retrograde motion (they move
    backwards compared to the direction the Sun
    moves).
  • Mercury and Venus are never seen at opposition
    (they always appear close to the Sun).

19
2.2 Greek Astronomy
  • Eratosthenes Measuring the diameter of Earth.

20
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    ???????? ?? ????? ?????? ????? (1973,2)
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    ?????? (0.3 ).

21
Al-Bairouni ????????
  • ???? ?? ????? ???????? ?? ????? ??? ????? !
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